Karl Gordon
Karl Gordon
Not sure. It's been too long. ;-)
Not sure. You can look in the kurucz subdir to see (physicsmodel/stars). The spectra look very different. Are these for the same log(g), Teff?
Putting the script into somewhere in physicsmodel/stars would be great. Hopefully named something descriptive.
Even normalized, the shapes are different. And you didn't say if they were for the same log(g),Teff.
The grid weights should be implemented like the new prior weights class (#649). The generic grid weight class should handle non-uniformly spaced grids including ones like the current variable width...
I think this has been answered as due to sources at the edges. But I'm not sure this has been tested. @cmurray-astro, @galaxyumi, @christinawlindberg, @lea-hagen or anyone else - have...
There are many fewer sources for sure. But I think I see a few of them in the F336W plot. I will send you the file (it is only 8.3...
Nice plots! Definitely says we should avoid edges. I wonder if there is some flag that says we are near the edge in the photometry files.
One idea would be to fit a small portion of the full catalog suitably picked to be representative of the full catalog (maybe 1%?) with physics grids of different resolutions....
I do think it is useful - thanks for opening this PR. I think it does require some documentation to explain the plots and what users should look for. Also,...